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The reason for this similarity is simple Learn how this process works, how the far side of the moon looks, and how it affects the moon's orbit and rotation. We almost always see the same surface when we stare at the moon, the same patterns of craters and cavities, thanks to the way that the moon moves, rotating and revolving around earth
So, what about the other surface of our only natural satellite? The answer lies in tidal locking, a gravitational phenomenon that causes the moon to always show the same face to earth Explore the fundamental astronomical reasons why we always see the same face of the moon
Understand this common celestial alignment.
The video shows how the moon's rotation and orbit are in sync with earth's, and how this creates the phenomenon of tidal locking It also reveals how the first images of the far side of the moon were taken in 1959 by luna 3. The moon is tidally locked to earth, meaning it rotates on its axis at the same speed as it orbits earth This results in the moon always showing the same face to earth, and explains the far side and dark side misconceptions.
The distinctive pattern of bright highlands and dark lunar maria on the moon has been turned towards us for millennia, visible to every human who has ever stood on earth But why do we only see this one side of the moon We know that earth spins about its axis, so why don't we get to see the full lunar surface as our moon does the same? The moon orbits earth in synchronous rotation, always keeping the same face toward us
Learn how humans have explored the nearside and farside of the moon with space missions and satellites.
Over billions of years, the earth's gravity has forced the moon to spin synchronously with its orbit However, things are a bit more complicated than that Viewed from earth, the moon appears to rock slowly backwards and forwards so that we see a slightly different face throughout the lunar month There are two main reasons for this.
The simple answer (and one that you've probably heard before) is that we only see one side of the moon because the moon rotates around the earth at the exact same speed as it rotates around its own axis, so that the same side of the moon is constantly facing the surface of the earth This means that one full 'day' of the moon (meaning the length of time it takes for the moon to rotate. In 1959, the soviet luna 3 probe provided the first images of this lunar hemisphere The moon's slight wobble while the moon largely keeps one face toward earth, we see slightly more than 50% of its surface over time due to libration
This slight wobble allows observers to glimpse about 59% of the moon's total surface.
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